Novae and Supernovae
Novae and supernovae are astronomical phenomena that captivate both amateur stargazers and seasoned astrophysicists alike. These cosmic events, characterized by the sudden and dramatic increase in brightness of a star, play significant roles in shaping our understanding of stellar evolution and the dynamics of the universe. Novae, often referred to as "new stars," occur in binary star systems when a white dwarf accretes matter from its companion star, triggering a thermonuclear explosion on its surface. In contrast, supernovae represent the cataclysmic death throes of massive stars, resulting in the release of staggering amounts of energy and the formation of exotic celestial remnants.
- Why are pulsars not always associated with supernova remnants?
- How can we see supernova remnant G1.9+0.3? If it is estimated to be about 25,000 light years away and now NASA says that it is about 140 years old, how can we even observe it? Wouldn't it still appear as a star to us for the next 24,860 years or so?
- What kind of star is most likely to become a white-dwarf supernova?
- What happens when a red giant star becomes a white dwarf?
- What kind of a star goes “nova” (not supernova)?
- Could our Sun ever undergo a nova or white dwarf supernova event? Why or why not?
- Would you expect to find supernova remnants inside globular clusters? Why?
- How long do supernova remnants last?
- Could a novae and a white dwarf supernova occur with a white dwarf that is not a member of a binary star system?
- What is the difference between astrophysics and astrobiology?
- Which books are good to get good knowledge in astrophysics?